On the Formation of the Most Massive Stars in the Galaxy
The most massive stars in the galaxy - those with more than 15 to 20 solar masses - are lilkely to ionize their surroundings before they reach their final mass. How can they accrete in spite of the presence of over-pressurized gas? This thesis presents results of Submillimeter Array (SMA) and Very L...
Clasificación: | Libro Electrónico |
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Autor principal: | Galván-Madrid, Roberto J. (Autor) |
Autor Corporativo: | SpringerLink (Online service) |
Formato: | Electrónico eBook |
Idioma: | Inglés |
Publicado: |
New York, NY :
Springer New York : Imprint: Springer,
2012.
|
Edición: | 1st ed. 2012. |
Colección: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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Temas: | |
Acceso en línea: | Texto Completo |
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